Zobrazeno 1 - 10
of 75
pro vyhledávání: '"Marton, Gabor"'
Autor:
Marton, Gábor, Gezer, Ilknur, Madarász, Máté, Dionatos, Odysseas, Audard, Marc, Roquette, Julia, Hernandez, David, Paladini, Roberta, Altieri, Bruno
Herschel operated as an observatory, therefore it did not cover the whole sky, but still observed ~8% of it. The first version of an overall Herschel/PACS Point Source Catalogue was released in 2017. The data are still unique and are very important f
Externí odkaz:
http://arxiv.org/abs/2406.03116
Autor:
Fiorellino, Eleonora, Abraham, Peter, Kospal, Agnes, Kun, Maria, Alcala, Juan M., Garatti, Alessio Caratti o, de Miera, Fernando Cruz-Saenz, Garcia-Alvarez, David, Giannini, Teresa, Park, Sunkyung, Siwak, Michal, Szilagyi, Mate, Covino, Elvira, Marton, Gabor, Nagy, Zsofia, Nisini, Brunella, Szabo, Zsofia Marianna, Bora, Zsofia, Cseh, Borbala, Kalup, Csilla, Krezinger, Mate, Kriskovics, Levente, Ogloza, Waldemar, Pal, Andras, Sodor, Adam, Sonbas, Eda, Szakats, Robert, Vida, Krisztian, Vinko, Jozsef, Wyrzykowski, Lukasz, Zielinski, Pawel
Publikováno v:
A&A 686, A160 (2024)
Context. Gaia18cjb is one of the Gaia-alerted eruptive young star candidates which has been experiencing a slow and strong brightening during the last 13 years, similar to some FU Orionis-type objects. Aims. The aim of this work is to derive the youn
Externí odkaz:
http://arxiv.org/abs/2403.08698
Autor:
Siwak, Michał, Hillenbrand, Lynne A., Kóspál, Ágnes, Ábrahám, Péter, Giannini, Teresa, De, Kishalay, Moór, Attila, Szilágyi, Máté, Janík, Jan, Koen, Chris, Park, Sunkyung, Nagy, Zsófia, de Miera, Fernando Cruz-Sáenz, Fiorellino, Eleonora, Marton, Gábor, Kun, Mária, Lucas, Philip W., Udalski, Andrzej, Szabó, Zsófia Marianna
Gaia21bty, a pre-main sequence star that previously had shown aperiodic dips in its light curve, underwent a considerable $\Delta G\approx2.9$ mag brightening that occurred over a few months between 2020 October - 2021 February. The Gaia lightcurve s
Externí odkaz:
http://arxiv.org/abs/2307.08802
Autor:
Nagy, Zsófia, Park, Sunkyung, Ábrahám, Péter, Kóspál, Ágnes, de Miera, Fernando Cruz-Sáenz, Kun, Mária, Siwak, Michał, Szabó, Zsófia Marianna, Szilágyi, Máté, Fiorellino, Eleonora, Giannini, Teresa, Lee, Jae-Joon, Lee, Jeong-Eun, Marton, Gábor, Szabados, László, Vitali, Fabrizio, Andrzejewski, Jan, Gromadzki, Mariusz, Hodgkin, Simon, Jabłońska, Maja, Mendez, Rene A., Merc, Jaroslav, Michniewicz, Olga, Mikołajczyk, Przemysław J., Pylypenko, Uliana, Ratajczak, Milena, Wyrzykowski, Łukasz, Zejmo, Michal, Zieliński, Paweł
FU Orionis objects (FUors) are eruptive young stars, which exhibit outbursts that last from decades to a century. Due to the duration of their outbursts, and to the fact that only about two dozens of such sources are known, information on the end of
Externí odkaz:
http://arxiv.org/abs/2307.01629
OB associations, birthplaces of the most luminous stars, are key objects for understanding the formation of high-mass stars and their effects on their environments. The aim of this work is to explore the structure and kinematics of the Cepheus OB2 as
Externí odkaz:
http://arxiv.org/abs/2301.02346
Autor:
Rimoldini, Lorenzo, Holl, Berry, Gavras, Panagiotis, Audard, Marc, De Ridder, Joris, Mowlavi, Nami, Nienartowicz, Krzysztof, de Fombelle, Grégory Jevardat, Lecoeur-Taïbi, Isabelle, Karbevska, Lea, Evans, Dafydd W., Ábrahám, Péter, Carnerero, Maria I., Clementini, Gisella, Distefano, Elisa, Garofalo, Alessia, García-Lario, Pedro, Gomel, Roy, Klioner, Sergei A., Kruszyńska, Katarzyna, Lanzafame, Alessandro C., Lebzelter, Thomas, Marton, Gábor, Mazeh, Tsevi, Molinaro, Roberto, Panahi, Aviad, Raiteri, Claudia M., Ripepi, Vincenzo, Szabados, László, Teyssier, David, Trabucchi, Michele, Wyrzykowski, Łukasz, Zucker, Shay, Eyer, Laurent
Publikováno v:
A&A 674, A14 (2023)
Gaia DR3 contains 1.8 billion sources with G-band photometry, 1.5 billion of which with BP and RP photometry, complemented by positions on the sky, parallax, and proper motion. The median number of field-of-view transits in the three photometric band
Externí odkaz:
http://arxiv.org/abs/2211.17238
Autor:
Kecskeméthy, Viktória, Kiss, Csaba, Szakáts, Róbert, Pál, András, Szabó, Gyula M., Molnár, László, Sárneczky, Krisztián, Vinkó, József, Szabó, Róbert, Marton, Gábor, Farkas-Takács, Anikó, Kalup, Csilla E., Kiss, László L.
The K2 mission of the Kepler Space Telescope allowed the observations of light curves of small solar system bodies throughout the whole Solar system. In this paper we present the results of a collection of K2 transneptunian object observations, betwe
Externí odkaz:
http://arxiv.org/abs/2210.06571
Autor:
Nagy, Zsófia, Ábrahám, Péter, Kóspál, Ágnes, Park, Sunkyung, Siwak, Michał, de Miera, Fernando Cruz-Sáenz, Fiorellino, Eleonora, García-Álvarez, David, Szabó, Zsófia Marianna, Antoniucci, Simone, Giannini, Teresa, Giunta, Alessio, Kriskovics, Levente, Kun, Mária, Marton, Gábor, Moór, Attila, Nisini, Brunella, Pál, Andras, Szabados, László, Zielinski, Paweł, Wyrzykowski, Łukasz
Young stars show variability on different time-scales from hours to decades, with a range of amplitudes. We studied two young stars, which triggered the Gaia Science Alerts system due to brightenings on a time-scale of a year. Gaia20bwa brightened by
Externí odkaz:
http://arxiv.org/abs/2207.02341
Autor:
Marton, Gábor, Ábrahám, Péter, Rimoldini, Lorenzo, Audard, Marc, Kun, Mária, Nagy, Zsófia, Kóspál, Ágnes, Szabados, László, Holl, Berry, Gavras, Panagiotis, Mowlavi, Nami, Nienartowicz, Krzysztof, de Fombelle, Grégory Jevardat, Lecoeur-Taïbi, Isabelle, Karbevska, Lea, Garcia-Lario, Pedro, Eyer, Laurent
Publikováno v:
A&A 674, A21 (2023)
Context. The Gaia third Data Release (DR3) presents the first catalogue of full-sky variable Young Stellar Object (YSO) candidates observed by the Gaia space telescope during the initial 34 months of science operations. Aims. Numerous types of variab
Externí odkaz:
http://arxiv.org/abs/2206.05796
Autor:
Szabó, Gyula M., Pál, András, Szigeti, László, Bognár, Zsófia, Bódi, Attila, Kalup, Csilla, Jäger, Zoltán J., Kiss, László L., Kiss, Csaba, Kovács, József, Marton, Gábor, Molnár, László, Plachy, Emese, Sárneczky, Krisztián, Szakáts, Róbert, Szabó, Róbert
Here we present the analysis of the distribution of rotation periods and light curve amplitudes based on 2859 family asteroids in 16 Main Belt families based on 9912 TESS asteroid light curves in the TSSYS-DR1 asteroid light curve database. We found
Externí odkaz:
http://arxiv.org/abs/2202.04372